SDO HMI 2014-04-07 16:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 80.44 | 402.18 | 44.22 | 221.14 | 12.83 | 13.44 | 17.45 | 317.62 | 0.4357 | -1145.6 | -380.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.41 | 0.00 | 0.77 | 10.95 | 14.27 | 18.28 | 313.15 | 0.4240 | -740.0 | -676.9 | |
| 46.47 | 383.85 | 25.54 | 211.08 | 12.57 | 13.68 | 17.69 | 316.82 | 0.4352 | -1553.9 | -415.4 | |
| 0.97 | -2.00 | 0.53 | -2.00 | 13.26 | 13.50 | 17.51 | 318.20 | 0.4412 | -668.1 | 999999 | |
| 23.68 | -2.00 | 13.01 | -2.00 | 12.93 | 13.22 | 17.23 | 318.15 | 0.4345 | -1316.4 | 999999 | |
| 0.00 | 2.38 | 0.00 | 1.29 | 10.56 | 13.03 | 17.04 | 314.49 | 0.4056 | 975.0 | 711.8 | |
| 0.00 | 2.38 | 0.00 | 1.32 | 14.66 | 13.29 | 17.30 | 320.63 | 0.4554 | 547.0 | 528.9 | |
| 5.63 | -2.00 | 3.10 | -2.00 | 13.28 | 13.12 | 17.12 | 318.86 | 0.4374 | -1032.0 | 999999 | |
| 2.55 | -2.00 | 1.41 | -2.00 | 14.14 | 13.18 | 17.19 | 320.05 | 0.4482 | -828.1 | 999999 | |
| 0.00 | 0.62 | 0.00 | 0.33 | 9.84 | 12.80 | 16.81 | 313.56 | 0.3949 | 700.0 | 576.7 | |
| 0.00 | 5.11 | 0.00 | 2.83 | 14.89 | 12.56 | 16.57 | 322.16 | 0.4511 | 837.0 | 685.6 | |
| 0.00 | 1.32 | 0.00 | 0.72 | 13.16 | 12.17 | 16.18 | 320.27 | 0.4264 | -207.0 | -196.2 | |
| 0.00 | 0.97 | 0.00 | 0.53 | 15.03 | 11.67 | 15.68 | 323.87 | 0.4444 | -626.0 | -486.2 | |
| 1.14 | 3.26 | 0.63 | 1.79 | 14.72 | 11.19 | 15.20 | 324.28 | 0.4363 | -921.8 | -728.8 | |
| 0.00 | 0.88 | 0.00 | 0.48 | 14.63 | 9.97 | 13.98 | 326.39 | 0.4240 | 803.0 | 648.5 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |